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handbook of modern sensors

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130 4 Optical Components <strong>of</strong> Sensors<br />

system. In any event, the so-called photometric characteristics <strong>of</strong> the optical system<br />

should be taken into account. Such characteristics include light, emittance, luminance,<br />

brightness, and so forth.<br />

To measure radiant intensity and brightness, special units have been devised.<br />

Radiant flux (energy emitted per unit time), which is situated in a visible portion <strong>of</strong> the<br />

spectrum, is referred to as luminous flux. This distinction is due to the inability <strong>of</strong> the<br />

human eye to respond equally to like power levels <strong>of</strong> different visible wavelengths.<br />

For instance, one red and one blue light <strong>of</strong> the same intensity will produce very<br />

different sensations; the red will be perceived as much brighter. Hence, comparing<br />

lights <strong>of</strong> different colors, the watt becomes a poor measure <strong>of</strong> brightness and a special<br />

unit called a lumen was introduced. It is based on a standard radiation source with<br />

molten platinum formed in a shape <strong>of</strong> a blackbody and visible through a specified<br />

aperture within a solid angle <strong>of</strong> one steradian. A solid angle is defined in a spherical<br />

geometry as<br />

ω = A r 2 , (4.13)<br />

where r is the spherical radius and A is the spherical surface <strong>of</strong> interest. When A = r,<br />

the unit is called a spherical radian or steradian (sr) (see Table 1.7).<br />

Illuminance is given as<br />

E = dF<br />

dA ; (4.14)<br />

that is, a differential amount <strong>of</strong> luminous flux (F ) over a differential area. It is most<br />

<strong>of</strong>ten expressed in lumens per square meter (square foot), or foot-meter (foot-candle).<br />

The luminous intensity specifies flux over solid angle:<br />

I L = dF<br />

dω ; (4.15)<br />

most <strong>of</strong>ten, it is expressed in lumens per steradian or candela. If the luminous intensity<br />

is constant with respect to the angle <strong>of</strong> emission, Eq. (4.15) becomes<br />

I L = F ω . (4.16)<br />

If the wavelength <strong>of</strong> the radiation varies but the illumination is held constant, the<br />

radiative power in watts is found to vary. A relationship between illumination and<br />

radiative power must be specified at a particular frequency. The point <strong>of</strong> specification<br />

has been taken to be at a wavelength <strong>of</strong> 0.555 µm, which is the peak <strong>of</strong> the spectral<br />

response <strong>of</strong> the human eye. At this wavelength, 1 W <strong>of</strong> radiative power is equivalent<br />

to 680 lumens. For the convenience <strong>of</strong> the reader, some useful terminology is given<br />

in Table 4.1.<br />

In the selection <strong>of</strong> electro-optical <strong>sensors</strong>, design considerations <strong>of</strong> light sources<br />

are <strong>of</strong> prime concern. A light source will effectively appear as either a point source<br />

or as an area source, depending on the relationship between the size <strong>of</strong> the source<br />

and the distance between the source and the detector. Point sources are arbitrarily<br />

defined as those whose diameter is less than 10% <strong>of</strong> the distance between the source

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